IC 2391
(MWSC 1529; FoF 2438; OCSN 204)
0.97
UTI
0.84
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
48.3 [arcmin]
- CN 0.84 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
IC 2391 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.
Very close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 130.302 | -53.015 | 6.606 | -24.741 | 23.324 | 14.412 |
| Li et al. | 2025 | 130.292 | -52.991 | 6.582 | -24.644 | 23.316 | â |
| Almeida et al. | 2025 | 130.382 | -53.001 | â | â | â | â |
| Alfonso et al. | 2024 | 130.301 | -53.023 | 6.592 | -24.764 | 23.371 | â |
| Hunt & Reffert | 2024 | 130.26 | -53.042 | 6.622 | -24.797 | 23.267 | 13.458 |
| Celli et al. | 2024 | 130.292 | -52.991 | â | â | â | â |
| Cavallo et al. | 2024 | 130.467 | -53.066 | 6.621 | â | â | â |
| Hunt & Reffert | 2023 | 130.26 | -53.042 | 6.622 | -24.797 | 23.267 | 13.458 |
| Almeida et al. | 2023 | 130.768 | -53.089 | â | â | â | â |
| Qin et al. | 2023 | 130.17 | -53.13 | 6.63 | -24.77 | 23.41 | 14.78 |
| Just et al. | 2023 | 130.061 | -53.025 | â | â | â | â |
| He et al. | 2022 | 130.332 | -53.057 | 6.613 | -24.786 | 23.33 | â |
| Jaehnig et al. | 2021 | 130.202 | -52.97 | 6.616 | -24.702 | 23.382 | â |
| Rain et al. | 2021 | 130.292 | -52.991 | 6.582 | -24.644 | 23.316 | â |
| Dias et al. | 2021 | 130.382 | -53.001 | 6.572 | -24.764 | 23.278 | 15.204 |
| Cantat-Gaudin et al. | 2020 | 130.292 | -52.991 | 6.582 | -24.644 | 23.316 | â |
| Cantat-Gaudin & Anders | 2020 | 130.292 | -52.991 | 6.582 | -24.644 | 23.316 | â |
| Liu & Pang | 2019 | 130.175 | -53.014 | 6.559 | -24.65 | 23.304 | â |
| Bossini et al. | 2019 | 130.292 | -52.991 | â | â | â | â |
| Soubiran et al. | 2018 | 130.292 | -52.991 | â | â | â | 15.29 |
| Cantat-Gaudin et al. | 2018 | 130.292 | -52.991 | 6.582 | -24.644 | 23.316 | â |
| Yen et al. | 2018 | 130.12 | -53.167 | 6.74 | -24.51 | 23.28 | â |
| Loktin & Popova | 2017 | 130.14 | -53.032 | â | -24.97 | 22.7 | 14.6 |
| Kharchenko et al. | 2016 | 130.061 | -53.025 | â | â | â | â |
| Dias et al. | 2014 | 130.133 | -53.033 | â | -3.23 | 4.07 | â |
| Kharchenko et al. | 2013 | 130.065 | -53.028 | â | -24.2 | 23.42 | 14.6 |
| Gozha et al. | 2012 | 130.133 | -53.033 | â | â | â | â |
| Piskunov et al. | 2008 | 130.143 | -53.026 | â | â | â | â |
| Kharchenko et al. | 2007 | 130.14 | -53.03 | â | 1.25 | â | 16.04 |
| Piskunov et al. | 2007 | 130.143 | -53.026 | â | â | â | â |
| van den Bergh | 2006 | 130.15 | -53.033 | â | â | â | â |
| Kharchenko et al. | 2005 | 130.14 | -53.03 | â | -24.19 | 23.48 | 16.04 |
| Kharchenko et al. | 2003 | 130.05 | -53.05 | â | -25.16 | 22.23 | â |
| Chen et al. | 2003 | 130.05 | -53.069 | â | â | â | â |
| Dias et al. | 2002 | 130.133 | -53.033 | â | -24.97 | 22.7 | 14.49 |
| Dambis | 1999 | 130.133 | -53.033 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.14 | 0.11 | â | 59 | -0.045 | â | â | â |
| Almeida et al. | 2025 | 0.15 | 0.16 | â | 49 | â | 139 | â | â |
| Alfonso et al. | 2024 | 0.15 | 0.04 | â | 40 | 0.001 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 169* | â | â |
| Celli et al. | 2024 | â | â | â | 29 | â | 160 | â | â |
| Cavallo et al. | 2024 | 0.15 | 0.49 | â | 45 | 0.160 | â | â | â |
| Hunt & Reffert | 2023 | 0.15 | 0.09 | 0.47 | 27 | â | â | â | â |
| Almeida et al. | 2023 | 0.15 | 0.09 | â | 58 | 0.124 | 215* | 0.22 | â |
| Qin et al. | 2023 | 0.16 | 0.19 | â | 40 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 112 | â | 5 | â | â |
| He et al. | 2022 | â | 0.40 | â | 63 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.15* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.15 | 0.09 | â | 36 | â | â | â | 0 |
| Dias et al. | 2021 | 0.15 | 0.16 | â | 49 | 0.000 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.15 | 0.04 | â | 29 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.15 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 41 | 0.000 | â | â | â |
| Bossini et al. | 2019 | 0.15 | 0.09 | â | 36 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.15 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.15 | â | â | â | â | â | â | â |
| Yen et al. | 2018 | 0.16 | 0.18 | â | 81 | â | â | â | â |
| Loktin & Popova | 2017 | 0.18 | 0.02 | â | 46 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.17 | 0.16 | â | 112 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.17 | 0.16 | â | 112 | -0.155 | â | â | â |
| Gozha et al. | 2012 | 0.17 | â | â | 46 | -0.010 | 93 | â | â |
| Piskunov et al. | 2008 | 0.18 | 0.03 | â | 76 | â | 284* | â | â |
| Piskunov et al. | 2007 | 0.18 | 0.03 | â | 76 | â | 175 | â | â |
| van den Bergh | 2006 | 0.17 | 0.03 | â | 46 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.18 | 0.03 | â | 76 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.15 | â | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.17 | 0.02 | â | 40 | -0.090* | â | â | â |
| Dias et al. | 2002 | 0.17 | 0.02 | â | 46 | -0.010 | â | â | â |
| Dambis | 1999 | 0.14 | 0.01 | â | 50 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.